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Fig. 2.

image

Top row: total horizontal turbulent diffusivity Dh (full line) and its Dh,v component (when active if Re > Re;c; dotted lines) for the 1.0 M, Z models described in Table 2 at three evolutionary stages (from left to right: ZAMS, age of the Sun, and when the central H mass fraction is reduced to 10% of its original value). The hatched areas correspond to the convective regions. Bottom row: vertical turbulent diffusion coefficient in the same models.

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